Re`nyi Holographic Dark Energy models in Teleparallel gravity
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Date
2022-07-06
Journal Title
Journal ISSN
Volume Title
Publisher
arXiv preprint arXiv
Abstract
In this paper, we have investigated the physical behavior of cosmological models in
the framework of modified Teleparallel gravity. This model is established using a Renyi
holographic “dark energy model (RHDE) with a Hubble cutoff. Here we have considered
a homogeneous and isotropic Friedman universe filled with perfect ‘fluid. The physical
parameters are derived for the present model in Compliances with 43 observational Hubble
data sets (OHD). The equation of state (EoS) parameter in terms of
H
(
z
) describes a
the transition of the universe between phantom and non-phantom phases in the context
of
f
(
T
) gravity. Our model shows the violation of strong energy condition (SEC) and the
weak energy condition (WEC) over the accelerated phantom regime. We also observed that
these models occupy freezing regions through
ω
D
−
ω
′D plane. Consequently, our Renyi
HDE model is supported to the consequences of general relativity in the framework of
f
(
T
)
modified gravity.
Description
Re`nyi Holographic Dark Energy models in Teleparallel gravity
Keywords
Citation
Bhardwaj, V.K., Dixit, A., Pradhan, A. and Krishannair, S., 2021. Rényi holographic dark energy models in teleparallel gravity. arXiv preprint arXiv:2109.12963.